“…However, the ionospheric day‐to‐day variability could still be influenced by nonlinear interaction of planetary waves and widely existed tides. Many studies have clearly identified ionospheric variations such as large perturbations of ion temperature (e.g., Goncharenko & Zhang, ), peak electron density ( f o F 2 ; e.g., Yue et al, ; Pancheva & Mukhtarov, ; Gupta & Upadhayaya, ), total electron content (e.g., Chau et al, ; Goncharenko et al, ; Goncharenko et al, ; Sridharan, ), equatorial electric field (e.g., Fejer et al, ), and equatorial electrojet (e.g., Sridharan et al, ) during SSW periods.…”